The Dark Matter Contribution to Galactic Diffuse Gamma Ray Emission
arXiv:1312.0006 · doi:10.1103/PhysRevD.89.063530
Abstract
Observations of diffuse Galactic gamma ray emission (DGE) by the Fermi Large Area Telescope (LAT) allow a detailed study of cosmic rays and the interstellar medium. However, diffuse emission models of the inner Galaxy underpredict the Fermi-LAT data at energies above a few GeV and hint at possible non-astrophysical sources including dark matter (DM) annihilations or decays. We present a study of the possible emission components from DM using the high-resolution Via Lactea II N-body simulation of a Milky Way-sized DM halo. We generate full-sky maps of DM annihilation and decay signals that include modeling of the adiabatic contraction of the host density profile, Sommerfeld enhanced DM annihilations, -wave annihilations, and decaying DM. We compare our results with the DGE models produced by the Fermi-LAT team over different sky regions, including the Galactic center, high Galactic latitudes, and the Galactic anti-center. This work provides possible templates to fit the observational data that includes the contribution of the subhalo population to DM gamma-ray emission, with the significance depending on the annihilation/decay channels and the Galactic regions being considered.
Published by PRD
References in corpus (10)
- A Theory of Dark Matter
- Dark matter and cosmic structure
- Constraining Light Dark Matter with Diffuse X-Ray and Gamma-Ray Observations
- A blueprint for detecting supersymmetric dark matter in the Galactic halo
- Constraints on the Galactic Halo Dark Matter from Fermi-LAT Diffuse Measurements
- The Dark Matter Annihilation Signal from Galactic Substructure: Predictions for GLAST
- The shapes, orientation, and alignment of Galactic dark matter subhalos
- Galactic Substructure and Dark Matter Annihilation in the Milky Way Halo
- Stringent Constraints On The Dark Matter Annihilation Cross Section From Subhalo Searches With The Fermi Gamma-Ray Space Telescope
- Constraints on WIMP Annihilation for Contracted Dark Matter in the Inner Galaxy with the Fermi-LAT